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Aerosol-Jet Printing - 5 microns to 5 millimeters.pdf
M3DAerosol-JetPrinting millimetersMichaelRenn, Ph.DDirector, M3D Applications LaboratoryAbout Optome
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Primary transit of the planet HD189733b at 3.6 and 5.8 microns.pdf
The hot Jupiter HD 189733b was observed during its primary transit using the nInfrared Array Camera on the Spitzer Space Telescope. The transit depths were nmeasured simultaneously at 3.6 and 5.8 microns. Our analysis yields values of n2.356 +- 0.019 % and 2.436 +- 0.020 % at 3.6 and 5.8 microns respectively, for na uniform source. We estimated the contribution of the limb-darkening and ns..
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4 Weiner S 1992 Bone structure from angstroms to microns.pdf
4 Weiner S 1992 Bone structure from angstroms to microns4 Weiner S 1992 Bone structure from angstroms to microns4 Weiner S 1992 Bone structure from angstroms to microns
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Camera for laser beam profiling from 1.0 to 2.0 microns wavelength with an indium gallium arsenide based focal plane array.pdf
LaserBeam Profiling from 1.0 2.0microns Wavelength IndiumGallium Arsenide based Focal Plane Array Ro
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BEPTHS BESS THAN TEN MICRONS Bavid L S tyx is.pdf
diffusioncoefficient metalsforpenetration depths less than ten microns Item type text; Thesis-Reprod
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Normalised flux + constant Wavelength (microns)归一化通量+恒波长(微米).pdf
Normalised flux + constant Wavelength (microns)归一化通量+恒波长(微米)
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Exoplanet Surveys at Five Microns with Direct and APP Imaging....pdf
Exoplanet Surveys at Five Microns with Direct and APP Imaging…
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The Wavelength Dependence of Interstellar Extinction from 1.25 to 8.0 microns Using GLIMPSE.pdf
The Wavelength Dependence of Interstellar Extinction from 1.25 to 8.0 microns Using GLIMPSE

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